2001/02/01 by John D. Barrow, John D Barrow, Yves Gaspar
Physics and Astronomy · #Asymptote #Black Holes and Theoretical Physics #Chaotic #Cosmological model #Cosmology #Cosmology and Gravitation Theories #Formalism (music) #Hamiltonian (control theory) #Initial singularity #Noncommutative and Quantum Gravity Theories #Singularity #astro-ph #gr-qc #hep-th
paper · pdf · doi:10.1088/0264-9381/18/9/314
published as Class.Quant.Grav. 18 (2001) 1809 · 22 pages, no figures, Latex file
arxiv created 2001/02/01 · openalex publication_date 2001/04/17 · arxiv updated 2009/11/30 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/06
Using a qualitative analysis based on the Hamiltonian formalism and the orthonormal frame representation we investigate whether the chaotic behaviour which occurs close to the initial singularity is still present in the far future of Bianchi VIII models. We describe some features of the vacuum Bianchi VIII models at late times which might be relevant for studying the nature of the future asymptote of the general vacuum inhomogeneous solution to the Einstein field equations.